Modeling mm- to X-ray flare emission from Sagittarius A*

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Table 2:

Delay times to the sub-mm/mm bands relative to the NIR/X-ray flare times as derived from our modeling.
Component	NIR/	340 GHz	43 GHz	Delay	Delay
	X-ray			340 GHz	43 GHz
$\alpha$	3.3	4	6	0.7	2.7
$\beta$	3.8	5.5	11.5	1.7	7.7
$\gamma$	8.3	9	13	0.7	4.7
$\delta$	10.4	11	16	0.6	5.6
$\epsilon$	1.6	2	9	0.4	7.4
$\zeta$	0.7	1	5	0.3	4.3
$\eta$	$\sim$ 9.0	10	15	1.0	6.0

Source LaTeX | All tables | In the text

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